To deal with surfaces and curves on them we start with a real, single-valued vector function and parametric angle variables using superscripts such that we have: u1 , u 2 , whence:
(1) x ( u1 , u 2 ) =
{ x 1 ( u1 , u 2 ), x 2 ( u1 , u 2 ) , x 3 ( u1 , u 2 ) }
With the two angular variables u1 , u 2 defined in a bounded domain B of the u1 u 2 -plane Then by equation (1) to any point ( u1 , u 2 ) in B there is associated in R 3 a point with position vector x (u1 , u 2). Then the point set in R 3 obtained when u1 , u 2 vary is called a parametric representation of the set and u1 , u 2 are the parameters of this representation.
In these
descriptions we will also make use of the Jacobian matrix of rank 2:
J =
(¶ x 1 /¶ u1 ¶ x 1 /¶ u 2 )
(¶ x 2 /¶ u1 ¶ x 2 /¶ u 2 )
(¶ x 3 /¶ u1 ¶ x 3 /¶ u 2 )
Partial derivatives of x ( u1 , u 3 ) can then be
denoted:
x 1 = ¶ x/ ¶ u1
And: x 13 = ¶ 2 x/ ¶ u1 ¶ u3
Which
can also be more generally denoted:
x a = ¶ x/ ¶ u1
And:
x ab = ¶ 2 x/ ¶ ua1 ¶ u b3
Or in the 2nd case:
x ab = ¶ 2 x/ ¶ u a¶ u b
Note there are three
determinants of 2nd order in the Jacobian J which bear
components of the vector products , i.e. of the vectors:
x 1 = ¶ x/ ¶ u1
and x 2 = ¶ x/ ¶ u2
These are different from the null vector IFF
x 1 and x 2 are linearly independent vectors
.
The assumption that the matrix for Jacobian
J is of rank 2 is thus the necessary and sufficient condition that said vectors
are linearly independent.
Note the x 1 x 2 -
plane can be represented in one of two forms, Cartesian:
(i)
x ( u1 , u 2 ) = (u1 , u 2, 0),
or polar
(ii)
x ( u1 , u 2 ) = ( u1 cos u 2 , u1 sin u 2, 0),
For which the respective
matrices are:
(i) J =
(1 ....0)
(0 ......1)
(0......0)
And (ii),
J =
( cos u 2 ,
-u1 sin u 2 )
( sin u 2 , u1 cos u 2 )
(0 .................... 0 )
Recall the sphere can be obtained by
extending the circle by one dimension ( x 2 ), i.e. to obtain:
x 3 = + Ö( r 2
- x 1 2 - x 2 2)
Depending on sign this is a representation of one of two hemispheres, x 3 > 0 or x 3 < o. The parametric angular representation of the preceding can be expressed:
x ( u1 , u 2 ) = (r cos u 2 cos u1, r
sin u 2 sin u1 , r
sin u 2)
or writing out in terms of x 1 , x 2 , x 3 .
x 1 = r cos u 2 cos u1, x 2 = r sin u 2 sin u1
x 3 = r sin u 2
The geometrical configuration is shown below:
The similarity to the celestial sphere of
astronomy will not be lost on many readers, i.e. the angular parameter u1 plays
an analogous role to Right Ascension while u 2 plays a role
analogous to the zenith distance (z) which is related to the coordinate of
declination ( d =
90 - z). Via this analogy we can also see the corresponding Jacobian matrix at
the poles is:
J
=
(-r cos u 2
sin u1 -r sin u 2 cos u1)
(r cos u 2
cos u1 -r
sin u 2 sin u1)
(0 .......................r cos u 2)
Example
2: A
cone of revolution with apex x= (0, 0 ,0) and with x 3 - axis as axis of
revolution i.e.
Can be represented in the form:
a ( x 12 + x 2 2) - x 32 = 0
And: x 3 = + a Ö(x 1 2 + x 2 2)
represents one of two graphics, x 3 > o and x 3 < 0 of the cone depending on the sign of the square root. In the case shown then we have; x 3 = aÖ(x 1 2 + x 2 2). The parametric representation can be written:
x ( u1, u 2 ) = ( u1 cos u2, u1 sin u 2 , au 2)
Note
the curves u1 =
const. are curves parallel to the x 1 x 2 - plane while the curves u1 =
const. are the generating straight lines of the cone.
Suggested Problems:
1) For the given cone of revolution (Example 2) write the corresponding Jacobian (matrix).
2) Find a parametric representation for each of the following:
a) Ellipsoid: x ( u1, u 2 ) = (a cos u2 cos u1 , b cos u2 sin u1, c sin u 2)
b) Hyperbolic paraboloid:
x ( u1 , u 2) = (au1 cosh u2, bu1 sinh u2, (u1 ) 2)
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